Gravitational question ( calculus )

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SUMMARY

The discussion focuses on calculating the time of collision (T) between two point masses, M1 and M2, separated by an initial distance r0, under gravitational attraction. The user applies fundamental physics equations, including F=ma and the gravitational force equation F=-GM1M2/r², to derive T in terms of M1, M2, G, and r0. The user encounters difficulties with integration while attempting to express T through the center of mass and conservation of energy principles, specifically in the integral T=R∫√(2GM2(1/r - 1/r0)) / (GM2/r²) dr.

PREREQUISITES
  • Understanding of Newton's laws of motion and gravitational force
  • Familiarity with calculus, particularly integration techniques
  • Knowledge of conservation of energy principles in physics
  • Concept of center of mass in a two-body system
NEXT STEPS
  • Study advanced integration techniques in calculus
  • Explore gravitational dynamics in two-body problems
  • Learn about the center of mass calculations in physics
  • Review conservation of energy applications in gravitational systems
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Students studying physics, particularly those focused on mechanics and gravitational interactions, as well as educators seeking to enhance their understanding of two-body collision problems.

peterpang1994
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Homework Statement


2 point mass M1 and M2 . Their separation is r0. They are released at rest at t=0. Find the time of collision (T)of them due to gravitational attraction in terms of M1, M2 , G and r0.

Homework Equations


F=ma
∫a(dt)2 = s (a is acceleration, s is displacement)
x0=(M2/(M1 + M2))r0 ( x is the position of center of mass respect to M1 )
F=-GM1M2/r2

The Attempt at a Solution


I used ∫a(dt)2 = s and make it becomes dt=(v/a)ds. As they should collide at the center of mass, the displacement of M1 should be equals to x. Therefore,
T=∫(v/a)dx
sup x=(M2/(M1 + M2))r , let (M2/(M1 + M2)) = R
x=Rr
dx=Rdr
T=R∫(v/a)dr (from r=r0 to r=0)
By law of conservation of energy,
(1/2)M1v2 = GM1M2(1/r - 1/r0)
v=√(2GM2(1/r - 1/r0))
a=GM2/r2
∴T=R∫√(2GM2(1/r - 1/r0)) / (GM2/r2) dr
After some calculation, I got
T=R√(2/(GM2r02))∫r2√(1/r - 1/r0)dr (from r=r0 to r=0)
I found that integration is very difficult. I wonder whether I get the correct direction or having conceptional and calculating error. I just hope that any help can be given. Thanks a lot.

Homework Statement


Homework Equations


The Attempt at a Solution

 
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